[89.06U] BIMA CO Observations of IRAS 07134+1005

IRAS 07134+1005 is a carbon rich proto-planetary nebula,
which is an evolved star object transitioning between the
asymptotic giant branch and planetary nebulae phases of
stellar evolution. Here, we present A,B,C and D array
observations of the CO J=1-0 line emission from IRAS
07134+1005 using the Berkeley-Illinois-Maryland Association
(BIMA) millimeter array. We resolve its molecular envelope
structure and compare it to the dust shell structures that
we have previously observed at mid-infrared and optical
wavelengths.

This work and Fong have been supported by NSF AST 99-81363
and Zalucha and Meixner have been also supported by NSF AST
97-33679.

The author(s) of this abstract have provided an email address
for comments about the abstract:
zalucha@uiuc.edu